activity
20182026
most citedA self-consistent semi-analytic model for Population III star formation in minihalos

31 citations · 55 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.GA2026

Searching for Population III stars with line intensity mapping cross-correlations

Sahil Hegde, Guochao Sun, Julian B. Muñoz +1

Decades of searches for Population III stars in individual galaxies have yielded a few potential candidates, but a statistically robust characterization of the demographics of the…

astro-ph.GA2026

Do we understand the star formation history of the universe?

Sahil Hegde, Steven R. Furlanetto, Smadar Naoz

The evolving relationship between a galaxy's mass and star formation rate -- the so-called `star-forming main sequence' (MS) -- provides a critical benchmark for understanding star…

astro-ph.GA2025★ 11 cited

Efficient semi-analytic modelling of Pop III star formation from Cosmic Dawn to Reionization

Sahil Hegde, Steven R. Furlanetto

The quest to find the first stars has driven astronomers across cosmic time, from hopes to identify their signatures in their heyday at cosmic dawn to deep searches for their remna…

astro-ph.GA2024★ 2 cited

A hidden population of active galactic nuclei can explain the overabundance of luminous objects observed by JWST

Sahil Hegde, Michael M. Wyatt, Steven R. Furlanetto

The first wave of observations with JWST has revealed a striking overabundance of luminous galaxies at early times () compared to models of galaxies calibrated to pre-JWST da…

astro-ph.CO2023★ 31 cited

A self-consistent semi-analytic model for Population III star formation in minihalos

Sahil Hegde, Steven R. Furlanetto

The formation of the first stars marks a watershed moment in the history of our universe. As the first luminous structures, these stars (also known as Population III, or Pop III st…

astro-ph.CO2023★ 4 cited

Modeling Strong Lenses from Wide-Field Ground-Based Observations in KiDS and GAMA

Shawn Knabel, B. W. Holwerda, J. Nightingale +13

Despite the success of galaxy-scale strong gravitational lens studies with Hubble-quality imaging, the number of well-studied strong lenses remains small. As a result, robust compa…

astro-ph.GA2022★ 3 cited

Reorientation Rates of Structural and Kinematic Axes in Simulated Massive Galaxies and the Origins of Prolate Rotation

Sahil Hegde, Greg L. Bryan, Shy Genel

In this work, we analyze a sample of 4000 massive ( at ) galaxies in TNG300, the box of the IllustrisTNG simulation suite…

astro-ph.SR2018★ 4 cited

Classifying Signatures of Sudden Ionospheric Disturbances

Sahil Hegde, Monica G. Bobra, Philip H. Scherrer

Solar activity, such as flares, produce bursts of high-energy radiation that temporarily enhance the D-region of the ionosphere and attenuate low-frequency radio waves. To track th…